Tech UPTechnologyTenth anniversary of the XMM-Newton telescope

Tenth anniversary of the XMM-Newton telescope

TheDecember 10, 1999, an Ariane 5 rocket took off from Kourou, French Guinea, carrying theXMM-Newton satellite, ten meters long. After several days of maneuvering, it reached its destination, an orbit one third of the way that separates us from the Moon. A few days later, XMM-Newton’s three gold-covered mirror modules began focusing X-rays on its five instruments. Since then, observations made with this telescope have served as the basis for the publication of 2,200 research articles.

TheX-raysthey are generated in space under the most extreme conditions, often as a result of tragic events. They can arise in the strong gravitational and magnetic fields that surroundneutron starso goblack holes, or train whenGiant gas clouds collide with galaxy clusters. The X-ray telescope has also played an important role in the study of thedark matter, a hypothetical substance that is supposed to be five times more abundant than normal matter. Closer to Earth, XMM-Newton has studied theice kitesand theMars atmosphere.

And it’s only the begining. “From a technological point of view,there is nothing that will not allow us to continue another decade“, concludes Norbert Schartel, head of this mission at the European Space Agency (ESA).

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Black holes
By identifying the X-rays emitted by iron atoms, the XMM-Newton telescope demonstrated how black holes twist the space-time fabric around themselves. It has also revealed how supermassive black holes grow and how they condition the evolution of the most massive galaxies in the Universe.

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Messier 82
Image of the galaxy Messier 82, also known asCigarette Galaxy. The image is composed of several different observations obtained by XMM-Newton of Messier 82, adding52.5 hours of total observation time. The center image shows plumes of hot X-ray glow gas emerging from the galactic disk (in blue), showing very intense star-forming activity.

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Stellar birth
This portrait of a star-forming cluster, calledNGC 346, is a combination of images obtained by XMM-Newton, NASA’s Spitzer Special Telescope and ESO (European Southern Observatory) ground-based telescopes.

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